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Timing neutron stars = pulsations, o...

Belloni, Tomaso M.

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Timing neutron stars = pulsations, oscillations and explosions /

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Timing neutron stars/ edited by Tomaso M. Belloni, Mariano Mendez, Chengmin Zhang.
其他題名:	pulsations, oscillations and explosions /
其他作者:	Belloni, Tomaso M.
出版者:	Berlin, Heidelberg :Springer Berlin Heidelberg : : 2021.,
面頁冊數:	xii, 335 p. :ill., digital ;24 cm.
內容註:	1. Astrophysical Constraints on Dense Matter in Neutron Stars -- 2. General Relativity Measurements from Pulsars -- 3. Magnetars: A Short Review and Some Sparse Considerations -- 4. Accreting Millisecond X-ray Pulsars -- 5. Thermonuclear X-ray Bursts -- 6. High-Frequency Variability in Neutron-Star Low-Mass X-ray Binaries.
Contained By:	Springer Nature eBook
標題:	Neutron stars. -
電子資源:	https://doi.org/10.1007/978-3-662-62110-3
ISBN:	9783662621103

Timing neutron stars = pulsations, oscillations and explosions /
Timing neutron starspulsations, oscillations and explosions /[electronic resource] :edited by Tomaso M. Belloni, Mariano Mendez, Chengmin Zhang. - Berlin, Heidelberg :Springer Berlin Heidelberg :2021. - xii, 335 p. :ill., digital ;24 cm. - Astrophysics and space science library,v.4610067-0057 ;. - Astrophysics and space science library ;v.461..

1. Astrophysical Constraints on Dense Matter in Neutron Stars -- 2. General Relativity Measurements from Pulsars -- 3. Magnetars: A Short Review and Some Sparse Considerations -- 4. Accreting Millisecond X-ray Pulsars -- 5. Thermonuclear X-ray Bursts -- 6. High-Frequency Variability in Neutron-Star Low-Mass X-ray Binaries.

Neutron stars, whether isolated or in a binary system, display a varied and complex phenomenology, often accompanied by extreme variability of many time scales, which takes the form of pulsations due to the object rotation, quasi-periodicities associated to accretion of matter, and explosions due to matter accreted on the surface or to starquakes of highly magnetized objects. This book gives an overview of the current observational and theoretical standpoint in the research on the physics under the extreme conditions that neutron stars naturally provide. The six chapters explore three physical regions of a neutron star: the space around it, where accretion and pulsar companions allow testing of general relativity its surface, where millisecond pulsation and X-ray bursts provide clues about general relativistic effects and the equation of state of neutron matter its interior, of course, inaccessible to direct observations, can nevertheless, be probed with all observational parameters related to neutron star variability.

ISBN: 9783662621103

Standard No.: 10.1007/978-3-662-62110-3doiSubjects--Topical Terms:

706876
Neutron stars.

LC Class. No.: QB843.N4 / T55 2021

Dewey Class. No.: 523.8874

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505 0 $a 1. Astrophysical Constraints on Dense Matter in Neutron Stars -- 2. General Relativity Measurements from Pulsars -- 3. Magnetars: A Short Review and Some Sparse Considerations -- 4. Accreting Millisecond X-ray Pulsars -- 5. Thermonuclear X-ray Bursts -- 6. High-Frequency Variability in Neutron-Star Low-Mass X-ray Binaries.
520 $a Neutron stars, whether isolated or in a binary system, display a varied and complex phenomenology, often accompanied by extreme variability of many time scales, which takes the form of pulsations due to the object rotation, quasi-periodicities associated to accretion of matter, and explosions due to matter accreted on the surface or to starquakes of highly magnetized objects. This book gives an overview of the current observational and theoretical standpoint in the research on the physics under the extreme conditions that neutron stars naturally provide. The six chapters explore three physical regions of a neutron star: the space around it, where accretion and pulsar companions allow testing of general relativity its surface, where millisecond pulsation and X-ray bursts provide clues about general relativistic effects and the equation of state of neutron matter its interior, of course, inaccessible to direct observations, can nevertheless, be probed with all observational parameters related to neutron star variability.
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